The nucleon source spectrum generating the muon component and expected coupling function for an inclined meson telescope

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Cosmic Rays, Energy Spectra, Muons, Nucleons, Particle Telescopes, Upper Atmosphere, Angular Distribution, Atmospheric Attenuation, Cascades, Mean Free Path, Mesons

Scientific paper

The nucleon spectrum at production is determined from direct measurements as well as indirect evidence, with a view toward its usefulness in the analysis of cosmic ray muon data from ground-based muon telescopes. The applicability of the Gross transformation is re-examined to obtain some information on the angular distribution of the nucleons. A fundamental study of a three-dimensional cascade is carried out for this purpose, since a linear cascade does not reflect the nucleon transport from one direction to another. A linear cascade approximation is shown to be useful in the derivation of muon monitor coupling functions. The expected coupling function for an inclined meson telescope with a zenith angle of 35 degrees is given.

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